Detection of β-Transitions in the Recombination Spectrum of Hydrogen near 9 cm Wavelength

Physics

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Scientific paper

THE detection in galactic emission nebulae of several of the hydrogen lines corresponding to transitions between levels with large principal quantum numbers has already been reported1-4. The lines were in the frequency range 8,873-1,424 Mc/s, corresponding to transitions in the range 90α-166α, using the notation suggested by Palmer and Zuckerman4 in which nα indicates a transition from level of quantum number (n+1) to n. A transition from (n+2) to n is indicated by nβ (see Fig. 1a).

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